SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 347, 401-408 (1999)


Table of Contents
Available formats: HTML | PDF | (gzipped) PostScript

Radiative losses of optically thin coronal plasmas

E. Landi and M. Landini

Department of Astronomy and Space Science, University of Florence, Italy

Received 9 March 1999 / Accepted 6 May 1999

Abstract

In the present work the total radiative losses and the total emissivity curve are calculated for an optically thin plasma using the Arcetri Spectral Code in the [FORMULA] temperature range. Checks have been made on the effects of changes in the parameters involved in the calculations, such as element abundances, ion fractions, electron density and transition probabilities on the resulting curves. Parametric fits are given for the resulting radiative losses curves and comparison is made with previous results.

Key words: plasmas – radiation mechanisms: non-thermal

Send offprint requests to: E.Landi (enricol@arcetri.astro.it)

© European Southern Observatory (ESO) 1999

Online publication: June 18, 1999

helpdesk.link@springer.de